Centre for Earth Evolution and Dynamics (CEED), Department of Geosciences, University of Oslo, Oslo, Norway.
Institut d'Astrophysique Spatiale, Université Paris-Sud, Orsay, France.
Astrobiology. 2021 Aug;21(8):997-1016. doi: 10.1089/ast.2020.2410.
Oxia Planum is a Noachian plain on Mars. It was chosen as the final landing site for studies by ExoMars 2022 rover. The main scientific objectives of the mission are to understand the mineralogy and aqueous evolution of ancient Mars with relevance to habitability. Oxia is covered by vast deposits of Fe,Mg-phyllosilicates, but the exact nature of these deposits is not yet fully understood. We performed a survey of potential terrestrial analog rocks, and here we show combined mineralogical characterization of these rocks with their near-infrared spectral analysis. Samples from two terrestrial sites were studied: (1) vermiculitized chlorite-schists from Otago, New Zealand, which underwent an alteration process without significant oxidation; and (2) basaltic tuffs from Granby, Massachusetts, USA, with Fe-rich clays filling amygdales of supposedly hydrothermal origin. Both analogues are incorporated into the newly built Planetary Terrestrial Analogue Library (PTAL) collection. Oxia bedrock clay-rich deposits are spectrally matched best by a well-crystallized trioctahedral vermiculite/saponite mixture from the basaltic tuff, although the contribution of saponite must be minor. Otago vermiculite is a good analogue to Oxia vermiculite in terms of overall mineralogy and Fe content. However, spectral inconsistencies related to the Al content in the Otago clays indicate that illitization of vermiculite, which results from postalteration oxidation, did not occur at Oxia. This implies limited water/rock interactions and reducing conditions during deposition of sediments now constituting the bedrock at Oxia. Whereas the spectral match does not conclusively imply the mineralogy, trioctahedral vermiculite should be considered a likely mineral component of the bedrock unit at Oxia Planum. Vermiculite has great potential to store organic matter, and the postdeposition geological context of Oxia Planum derived from understanding of environmental conditions in analog sites is promising for organic matter preservation.
乌托邦平原是火星上的一个诺亚纪平原。它被选为 2022 年 ExoMars 漫游车进行研究的最终着陆点。该任务的主要科学目标是了解火星古代的矿物学和水的演化过程,这与可居住性有关。乌托邦平原被大量的 Fe、Mg 层状硅酸盐所覆盖,但这些沉积物的确切性质尚未完全了解。我们对潜在的地球类似物岩石进行了调查,在此,我们展示了这些岩石的矿物学综合特征及其近红外光谱分析。研究了两个地球地点的样本:(1) 来自新西兰奥塔哥的蒙脱石-绿泥石片岩,经历了无明显氧化的蚀变过程;(2) 来自美国马萨诸塞州格兰比的玄武质凝灰岩,富铁粘土填充了据称是热液起源的杏仁体。这两个类似物都被纳入了新建立的行星地球类似物库(PTAL)中。乌托邦平原基岩粘土富积层的光谱与玄武质凝灰岩中结晶良好的三八面体蒙脱石/皂石混合物最佳匹配,尽管皂石的贡献必须较小。从整体矿物学和铁含量来看,奥塔哥蒙脱石是乌托邦平原蒙脱石的良好类似物。然而,与奥塔哥粘土中 Al 含量有关的光谱不一致表明,在奥塔哥粘土中发生的蒙皂石伊利石化没有发生在乌托邦平原,这表明水/岩石相互作用有限,并且在沉积现在构成乌托邦平原基岩的沉积物时,条件为还原。虽然光谱匹配并不能确定矿物学,但三八面体蒙脱石应该被认为是乌托邦平原基岩单元的一个可能的矿物成分。蒙脱石具有储存有机物的巨大潜力,从类似物站点的环境条件中得出的乌托邦平原的沉积后地质背景对于有机物的保存是有希望的。